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Fig. 11


Rest frame SED of the radio galaxies 3C324 (top) and 3C 356 (bottom). Data are from NED, Spitzer/IRS (Leipski et al. 2010) and Herschel (Podigachoski et al. 2015). A fit using a pure AGN is shown on the left and for a combination (black line) of AGN (red line) and starburst (blue dashed) activity on the right. Stellar light from the host (yellow dots) is added to better match the near-IR. Model parameters are given in Table 3.

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